... Brown University - Vernadsky Institute Microsymposium 38, October 27-29, 2003, Moscow, Russia . ... Michael G. G., European Space Agency, Research and Scientific Support Department, ESA/ESTEC, Noordwijk, The Netherlands, greg.michael@esa.int . ... 2Sternberg Astronomical Institute, Moscow, greg.michael@esa.int . ... Brown University - Vernadsky Institute Microsymposium 40, 2004, Moscow, Russia . ... Brown University - Vernadsky Institute Microsymposium 42, October 10-12, 2005, Moscow, Russia . ...

ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Information & tools for observers . ... Australia Telescope Online Archive (ATOA) . ... ATCA | ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... The Australia Telescope National Facility Colloquium . ...

We have studied the relationship between the star formation rate (SFR), surface density, and gas surface density in the spiral galaxy M51a (NGC 5194), using multiwavelength data obtained as part of the Spitzer Infrared Nearby Galaxies Survey (SINGS). ... The combination of these extinction-corrected SFR densities with aperture synthesis H I and CO maps has allowed us to probe the form of the spatially resolved star formation law on scales of 0.5-2 kpc. ...

... Michael E. Lopez-Alegria (Captain, USN, RET.) ... After his second mission, he led the International Space Station (ISS) Operations branch of the Astronaut Office. ... In October 2014 Lopez-Alegria became an independent consultant; he is based in Washington, D.C. SPACE FLIGHT EXPERIENCE: Mission Specialist (MS)-2, STS-73 Columbia (October 20 to November 5, 1995). ... The primary mission objective was delivery of the Expedition 6 crew to the ISS and the return of the Expedition 5 crew to Earth. ...

... T2042 Date Received: 2005-Jan-12 14:35:48 Technical Page Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Urgent Terrestrial Aeronomy Radar Ionosphere 36 Hours Helium Ion Layer Formation During Equinox The advent of improved light ion partitioning in the analysis of Arecib o Observatory Incoherent Scatter Radar (ISR) data has led to a renewed interest in the measurement and study of He+ ions. ... Part of the observing run. ...

Next: Low-Mass Star Formation Up: M.D. Smith Previous: M.D. Smith Contents . Massive stars are of elevated importance in our Universe for several reasons. ... During their lives, they influence the nurseries in which new stars might form. ... He and Michael Smith investigated the consequences of massive star formation in one such region of our Galaxy. They uncovered that massive stars are forming in the Rosette Molecular Complex at a rate way beyond previous expectations. ...

... Chapman and Ferraro (1931, 1932) were first to discuss the existence of a boundary to the Earth's magnetic field. During 1950's, as the concept of continuous solar wind emerged, it was obvious that such a feature should be a permanent feature of the magnetosphere . ... At this location, typically around 8 - 11 Re away on the Earth - Sun line, a large scale duskward (Chapman-Ferraro) current develops in the dayside magnetopause to cancel the Earth's field outside. ... Res., ...

... Ancient Layered Rocks on Mars . ... Credit: Malin Space Science Systems , MOC , MGS , JPL , NASA Explanation: Is this a picture of Mars or Earth? ... What may appear to some as a terrestrial coastline is in fact a formation of ancient layered rocks and wind-blown sand on Mars. The above-pictured region spans about three kilometers in Schiaparelli Crater . ... Publications with keywords: layered rocks - Mars . Publications with words: layered rocks - Mars . ... Victoria Crater on Mars . ...

... 2008 October 6 . Layers of Red Cliffs on Mars . Credit: HiRISE , MRO , LPL (U. Arizona) , NASA . Explanation: How did these layers of red cliffs form on Mars? No one is sure. The northern ice cap on Mars is nearly divided into two by a huge division named Chasma Boreale . ... Pictured above , several dusty layers leading into this deep chasm are visible. Cliff faces , mostly facing left but still partly visible from above , appear dramatically red. ... About APOD | ...

Confirmed Participants . ... Participants . ... Last updated:10:54:49 17-Jun-2015 . ...

. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .

... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members . ... Science Users Information . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ... ESO astronomers often are working on scientific programmes and data sets that are suited for PhD theses. This page gives an overview over what is currently offered by Faculty astronomers. ... Thesis topic . ...

Next: Functionality Up: RGS_QUANTUMEF Previous: RGS_QUANTUMEF Contents . This is one of the most important RGS calibration files, whose separate extensions describe different aspects of the physical model of the ensemble of gratings and CCD detectors that form an RGS instrument: . CCD_DESC . Thickness of CCD layers of passive material. ... Total thickness of CCDs including CCD_DESC dead layers. ... Michael Smith 2011-09-20 ...

Organisateurs: Michel Balazard (CNRS, Laboratoire Poncelet) , Michael Tsfasman (CNRS, Laboratoire Poncelet, Institut des Probl mes de Transmission de l'Information) , Alexey Zykin (Laboratoire Poncelet, Haute Ecole d'Economie) . ... Le laboratoire franco-russe Poncelet organise la troisi me conf rence "Zeta functions" du 21 au 25 juin 2010 l'Universit Ind pendante de Moscou. ... La conf rence portera essentiellement sur les avanc es les plus r centes dans le domaine des fonctions z ta. ...

Recent molecular observations indicate supersonic cloud-cloud collision is one of the important modes of O star formation. The O star formation regions studied so far include super star clusters (Westerlund2, NGC3603, RCW38 etc.), mini-starbursts (NGC6334, NGC6357 etc.) HII regions (M42/43, M20 etc.), and Spitzer bubbles (RCW120 etc.) ... Since the collision time scale is short ~10^5 yrs, O star formation is a rapid process with a mass accretion rate higher than 10^-4Mo/yr. ...

.

... Доклады предсталенные во время летней школы 'Atmosphere researches. Challenge for Ukraine", прошедшей с 15 по 19 сентября 2008 г. за поддержки Швейцарского национального научного фонда (JRP #?В7320-110831) . ... Introduction into Particulate matter research: Measurement techniques, formation, influence on air quality and climate. ... Ozone formation in the troposphere: Basic mechanisms and photooxidant air pollution. ... Atmosphere researches. Challenge for Ukraine' . ... 380(44)5264539 . ...

. Proceedings of Turbulent Shear Flows XI, Sept. 1997. Jacques Lewalle, jlewalle@syr.edu

Numerical simulation of electromagnetic scattering by morphologically complex objects Janna M. Dlugach*, Michael I. Mishchenko** *Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Kyiv, Ukraine **NASA Goddard Institute for Space Studies, New York, USA Radiation mechanisms of astrophysical objects: classics today 21 ­ 25 September, 2015, St.Petersburg. ... Phase angle dependence of the degree of linear polarization for the center of the Jovian disk. ...

sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...